de Bergh C, Bézard B, Owen T, Crisp D, Lutz B L
Département de Recherche Spatiale, Observatoire de Paris, Meudon, France.
Science. 1991 Feb 1;251:547-9. doi: 10.1126/science.251.4993.547.
Absorption lines of HDO and H2O have been detected in a 0.23-wave number resolution spectrum of the dark side of Venus in the interval 2.34 to 2.43 micrometers, where the atmosphere is sounded in the altitude range from 32 to 42 kilometers (8 to 3 bars). The resulting value of the deuterium-to-hydrogen ratio (D/H) is 120 +/- 40 times the telluric ratio, providing unequivocal confirmation of in situ Pioneer Venus mass spectrometer measurements that were in apparent conflict with an upper limit set from International Ultraviolet Explorer spectra. The 100-fold enrichment of the D/H ratio on Venus compared to Earth is thus a fundamental constraint on models for its atmospheric evolution.
在金星暗面2.34至2.43微米区间、波数分辨率为0.23的光谱中检测到了HDO和H₂O的吸收线,该区间探测的大气高度范围为32至42千米(8至3巴)。所得氘氢比(D/H)的值是地球值的120±40倍,明确证实了先锋金星号原位质谱仪的测量结果,该结果曾明显与国际紫外探测仪光谱设定的上限相冲突。因此,金星上D/H比相对于地球的100倍富集是其大气演化模型的一个基本限制条件。